object

axion

An axion is a hypothetical particle proposed as a candidate for dark matter.
38 related articles · 5 formulas · 6 who worked here

Description

The axion is a light particle predicted to solve the problem of CP violation in the strong interaction (why quarks behave symmetrically under mirror reflection). It hardly interacts with matter and could constitute cold dark matter. The search is conducted by attempting to convert an axion into a photon under the influence of a strong magnetic field.

History

The Peccei-Quinn mechanism was published in 1977, and soon Frank Wilczek and Steven Weinberg independently predicted a light boson. Wilczek named it the axion, by analogy with a cleaning agent that 'cleans up' QCD from the strong CP problem. In the 1980s, the first experiments were proposed, including a 'magnetic sequester.' In the 21st century, axion searches have become one of the main directions of particle physics, intertwined with astrophysics and cosmology.

How it works

The axion field a(x) interacts with electromagnetism through the term (g_{aγγ}/4) a F_{μν} ilde{F}^{μν} in the Lagrangian. In an external magnetic field, this leads to the conversion of axions into photons. Cosmologically, axions are born at the spontaneous breaking of symmetry, and their field is frozen until the moment when the mass becomes comparable to the Hubble rate; then it begins to oscillate, behaving as cold dark matter. For detection, resonance in microwave cavities is used (frequency is related to the axion mass) with sensitivity g_{aγγ} ~ 10^{-16} GeV^{-1}.

In practice

The search for axions is underway in dozens of laboratories using sensitive detectors and powerful magnets; their discovery will decipher the nature of dark matter and open the way to new physics.

Fun fact

An axion could shine through a solid lead wall a light-year thick without even noticing it.

Concept graph →

Formulas

$$l_{\rm osc} \propto \frac{\sqrt{1+(E_c/E_\gamma)^2}}{B_\perp g_{a\gamma}}$$
Length scale for periodic axion-photon conversion probability modulation.
What is in the formula
l_oscvariableOscillation length — length metre
E_cvariableCritical energy — energy joule
E_γvariablePhoton energy — energy joule
B_perpvariablePerpendicular magnetic field strength — magnetic field strength tesla
g_aγvariableAxion-photon coupling constant — coupling constant inverse gev
l_{\rmosc}=32{\rmкпк}\sqrt{1+(e_c/e_γ)^2}(\frac{b_\perp}{μ{г}})^{-1}(\frac{g_{aγ}}{10^{-11}{гэв}^{-1}})^{-1} · 2607.07158
$$q = Z/X$$
Axis ratio is height divided by length.
What is in the formula
qvariableAxis ratio — axis ratio
ZvariableHeight (vertical extent) — length metre
XvariableLength (horizontal extent) — length metre
q_{\rmdm}=z/x · 2510.08684
$$m_a \propto \frac{1}{f_a}$$
The axion mass is inversely proportional to the symmetry breaking scale.
What is in the formula
m_avariableAxion mass — mass kilogram
f_avariableAxion decay constant (symmetry breaking scale) — energy joule
∝operatorIndicates a direct proportionality relationship — proportionality
m_a\simeq5.7μ{эв}*\frac{10^{12}{гэв}}{f_a} · 2606.07742v1
m_a\approx5.7μ{ev}*\frac{10^{12}{gev}}{f_a} · 2607.23140v1
$$\operatorname{proj}_{\Delta^{K-1}}(\mathbf{z}) = \arg\min_{\mathbf{p} \in \Delta^{K-1}} \|\mathbf{p} - \mathbf{z}\|^2$$
Projects a vector onto the probability simplex with sparsity.
What is in the formula
zvariableInput vector to be projected — vector
pvariableProjected vector on the simplex — vector
projoperatorFinds the closest point in the simplex to the input vector — projection operator
argminoperatorReturns the value that minimizes the expression — argmin operator
‖·‖operatorComputes the square root of the sum of squares — euclidean norm
\operatorname{sparsemax}({z})=\arg\min_{{p}\inδ^{k-1}}\|{p}-{z}\|^2 · 2607.00004
$$\theta_{a,0} = \frac{g_{a\gamma}}{2} \frac{\sqrt{2\rho}}{\mu}$$
Amplitude of axion-induced polarization oscillations.
What is in the formula
\theta_{a,0}variableAmplitude of polarization oscillation — angle radian
g_{a\gamma}variableAxion-photon coupling constant — coupling constant reciprocal gev
\rhovariableLocal axion dark matter density — mass density kilogram per cubic metre
\muvariableAxion mass — mass kilogram
θ_{a,0}=\frac{g_{aγ}}{2}\frac{\sqrt{2ρ}}{μ} · 2607.04550v1

Related articles · 118

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The Invisible Conductor of a Pulsar: How an Axion Mane Makes a Dying Star Sing
The orchestra plays, though no one sees the conductor. The musicians are charged particles in the pulsar's magnetosphere, and the score is the electric and magnetic fields generated by the spinning superdense star.
A Deep Moat Around the Resonator: How to Catch an Axion in a Strong Field
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